A low-energy core-collapse supernova without a hydrogen envelope View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2009-06

AUTHORS

S. Valenti, A. Pastorello, E. Cappellaro, S. Benetti, P. A. Mazzali, J. Manteca, S. Taubenberger, N. Elias-Rosa, R. Ferrando, A. Harutyunyan, V. P. Hentunen, M. Nissinen, E. Pian, M. Turatto, L. Zampieri, S. J. Smartt

ABSTRACT

A supernova with a pastTheory suggests that stars with initial masses greater than 25–30 times that of the Sun end their stellar lives as Wolf–Rayet stars, becoming hydrogen-deficient by rapidly losing mass through strong stellar winds. Any subsequent supernova explosion should produce ejecta of low kinetic energy and faint optical luminosity, with a small mass fraction of radioactive nickel. Until now no core-collapse supernovae fitting this description have been detected. But SN 2008ha, discovered on 7 November 2008, appears to fit the bill. A detailed photometric and spectroscopic study shows SN 2008ha to be the faintest and lowest-luminosity hydrogen-deficient supernova known. This discovery raises the possibility that other similar events have been observed previously — SN 2002cx is one candidate — but were classified as 'peculiar thermonuclear supernovae'. More... »

PAGES

674-677

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature08023

DOI

http://dx.doi.org/10.1038/nature08023

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1053428733

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/19494909


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